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Chapter 16 – Atomic Energy - PowerPoint PPT Presentation

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Chapter 16 – Atomic Energy
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  1. Chapter 16 – Atomic Energy

  2. Section 1 Radioactivity • Terms to Learn • Nuclear radiation • Radioactivity • Radioactive Decay • Alpha Decay • Mass Number • Beta Decay • Isotopes • Gamma Decay • Half Life

  3. Discovering Radioactivity • Becquerel discovered radiation in 1896 – he was originally testing for UV light to leave an image on a photo plate but even without the light the rock was given off energy. • He figured this was due to the plutonium in the rock • This is nuclear radiation – high energy particles and rays that are emitted by the nuclei of some atoms • Radioactivity is the ability to give off nuclear energy (Marie Curie)

  4. Nuclear radiation is produced through Decay • Radioactive decay is the process in which the nucleus of a radioactive atom releases nuclear radiation • Three types of radioactive decay are • Alpha decay • Beta decay • Gamma decay

  5. Alpha Decay • Alpha Decay – the release of an alpha particle from a nucleus • Alpha particle consists of two protons and two neutrons • This means it has a mass number of 4 and a charge of 2+ • Remember mass number is the sum of the protons and the neutrons in an atom • All decay shares two characteristics • The mass number is conserved- the mass number of the reactants equals the mass number of the products • The charge is conserved – The sum of the charges of the reactants equals the sum of the charges of the products

  6. Beta Decay • Beta decay is the release of a beta particle • Can be either an electron (having a charge of 1- and a mass of almost 0) or a positron (having a charge of 1+ and a mass of almost 0) • Because electrons and positrons do not contain protons or neutrons the mass number of a beta particle is 0

  7. Two types of Beta Decay • Carbon -14 nucleus undergoes beta decay. During decay a neutron breaks into a proton and an electron. Nucleus becomes a nucleus of a different element. Mass number and charge are conserved. • Isotopes are atoms that have the same number of protons but different numbers of neutrons.

  8. Example • A carbon -11 nucleus undergoes beta decay when a proton breaks into a positron and a neutron. However, the beta decay of carbon-11 still changes the nucleus into a nucleus of a different element while conserving both mass number and charge.

  9. Gamma Decay • Energy is released during alpha decay and beta decay. Some of this energy is in the form of gamma rays, a form of light with very high energy. • Gamma decay is the release of gamma rays from a nucleus • Gamma decay occurs after alpha and beta decay as the particles in the nucleus shift to a more stable arrangement • Because gamma rays have no mass or charge, gamma decay alone does not cause one element to change into another as do alpha decay and beta decay

  10. Power of radiation • There are three forms of nuclear radiation that differ in their ability to penetrate (go through) matter • Alpha particles have the greatest charge and mass. They travel about 7cm through air and are stopped by paper or clothing. • Beta particles have a 1- or 1+ charge and almost no mass. That are more penetrating than alpha particles. They travel about 1 m through the air, but are stopped by 3mm of aluminum. • Gamma rays have no charge or mass and are the most penetrating. They are blocked by very dense, thick materials, such as a few centimeters of lead or a few meters of concrete.

  11. Effects of radiation on matter • Radiation can break chemical bonds between atoms. It can also knock electrons out of atoms. Both can cause damage living and non living things. • Cells can be damaged by radiation. Causes burns, can cause radiation sickness, and cancer. • Nonliving things can be hurt, metal can be weakened, space vehicles

  12. Damage at different depths • Gamma rays are the most penetrating and cause damage deep within while beta rays cause damage slightly more shallow. Alpha rays are the most shallow but because they are the largest and most massive radiation they cause the most damage.

  13. Nuclei decay to become stable • All nuclei composed of more than 83 protons are radioactive, this is because the force of attraction that holds a nucleus together is strong but only for a short distance. They may exist for billions of years but eventually decay and are therefore unstable. Too many protons

  14. Ratio of neutrons to protons can also make a nuclei unstable. • If it contains too many or too few neutrons compared to protons

  15. How does a nuclei become stable • An unstable nuclei will give off (emit) nuclear radiation until it has a stable number of protons and neutrons • Sometimes it takes more than one decay to become stable

  16. Finding a date by decay • Carbon-14 – Carbon atoms are found in all living things. A small percentage of these are carbon 14 radioactive atoms. During life the atoms are replaced but when you die they atoms are no longer replaced and they slowly decay.

  17. Decays Occur at a steady rate • Every 5,730 years half of the carbon 14 in a sample decays. The rate of decay is constant and is not affected by other conditions • Each radioactive isotope has its own rate of decay called a half life • Half life is the amount of time it takes for one half of the nuclei of a radioactive isotope to decay

  18. Determining age • The iceman’s age was determined by measuring the number of decays each minute. • Carbon 14 can be used to date things up to 50,000 years old • Anything past that you would need to use another element like potassium 40 which has a half life of 1.3 billion years

  19. Radioactivity and your world • Tracers- can be used to follow elements through paths • Used by doctors to find and kill cancer cells • Used to power space probes • Farmers can use it to trace what elements plants take in

  20. Section 2 – Energy from the Nucleus • Terms to Learn • Nuclear fission • Nuclear chain reaction • Nuclear fusion

  21. Nuclear Fission • Not all unstable nuclei decay by releasing an alpha or beta particle or gamma rays. Some decay by breaking down into two smaller, more stable nuclei during nuclear fission. • Nuclear fission is the process in which a large nucleus splits into two smaller nuclei with the release of energy.

  22. Energy from matter • You can get matter from energy. It is a tiny amount but the amount of material is tiny as well. • Nuclear chain reactions – a continuous series of nuclear fission reactions • Energy from a chain reaction – an uncontrolled chain reaction can produce a huge amount of energy such as an atomic bomb.

  23. Nuclear versus fossil fuel • Nuclear power plants are more expensive to build than fossil fuel plants but they are less expensive to operate because less fuel is needed

  24. Nuclear power plants • Nuclear power also does not release gases such as carbon dioxide however uranium is also a limited resource. • Nuclear power plants supply about 20 percent of the U.S. power

  25. Problems with Nuclear energy • Chernobyl – April 26, 1986 – Explosion reached almost all of Europe, Asia and even reached the US. • Nuclear waste – All the spent rods, covers the workers wear and even the chemicals will emit radiation for thousands of years.

  26. Nuclear Fusion • Another reaction where matter is converted to energy is nuclear fusion • Nuclear fusion is where two or more nuclei with small masses are joined together, or fuse, to form larger more massive nucleus. • The sun is the best source of nuclear fusion where hydrogen fuse together to form helium.

  27. Nuclear fusion • We cannot contain hydrogen plasma and it requires as more energy to contain plasma than energy that fusion would create. • The fuel for fusion is pretty much unlimited as there is lots of hydrogen in the ocean • Less concern over an accident because even with an explosion little radioactivity would be released. There is also much less waste.